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SPH simulations of star/planet formation triggered by cloud-cloud collisions

Published online by Cambridge University Press:  01 October 2007

Spyridon Kitsionas ,
Anthony P. Whitworth  and
Ralf S. Klessen
Spyridon Kitsionas
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany email: skitsionas@aip.de
Anthony P. Whitworth
Affiliation:
School of Physics & Astronomy, Cardiff University, P.O. Box 913, CF24 3AA Cardiff, U.K.
Ralf S. Klessen
Affiliation:
Institut für Theoretische Astrophysik, Universität Heidelberg, Albert-Ueberle-Str. 2, D-69120 Heidelberg, Germany
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Abstract

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We present results of hydrodynamic simulations of star formation triggered by cloud-cloud collisions. During the early stages of star formation, low-mass objects form by gravitational instabilities in protostellar discs. A number of these low-mass objects are in the sub-stellar mass range, including a few objects of planetary mass. The disc instabilities that lead to the formation of low-mass objects in our simulations are the product of disc-disc interactions and/or interactions between the discs and their surrounding gas.

Keywords

hydrodynamicsmethods: numericalstars: formationplanetary systems: protoplanetary disksplanetary systems: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S249: Exoplanets: Detection, Formation and Dynamics , October 2007 , pp. 271 - 278
Copyright
Copyright © International Astronomical Union 2008

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